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High Resolution ALMA Imaging of Arp 220 and Evolution of the ISM and Star Formation in the Early Universe
Wednesday, May 18, 2016 - 3:30pm to 4:30pm PDT
N232, Room 103
The new Atacama Large Millimeter Array (ALMA) consists of 64 high frequency mm/submm telescopes located in Northern Chile at 16,500 ft. It has now been in operation four years. I will present new imaging of the UltraLuminous IR galaxy Arp 220 at 90 mas resolution and our survey of interstellar gas contents of galaxies in 150 galaxies at z = 1 to 4.